Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • WEAVE monitoring of stellar clusters with O stars
    The MONOS project has obtained WEAVE LIFU observations to study the cores of nine stellar clusters containing O and B stars. Most O stars form in multiple systems, which allows for the determination of stellar masses through their orbits. However, this process is complicated by the wide range of orbital periods and the presence of complex systems
    Holgado, G. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • WEAVE first science
    WEAVE, the powerful multi-object spectrograph recently installed on the William Herschel Telescope (WHT), started science observations in October 2023. Over 500 hours of science observations have been taken with the Large Integral Field Unit (LIFU) mode in the first ∼10 months of observations, sharing nights with further technical and commissioning
    Balcells, M.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Vortex Flows in the Solar Atmosphere: Detection and Heating Mechanisms in 3D MHD Numerical Simulations
    Vortex flows are structures associated with the rotation of the plasma and/or the magnetic field that are present throughout the solar atmosphere. In recent years, their study has become increasingly important, as they are present on a wide variety of temporal and spatial scales and can connect several layers of the solar atmosphere. In this work
    Koll Pistarini, M. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Very high-energy gamma-ray detection and long-term multiwavelength view of the flaring blazar B2 1811+31
    Context. Among the blazars whose emission has been detected up to very high-energy (VHE; 100 GeV
    Abe, K. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Very First Approach to the Lack of Fast Rotators in Cygnus OB2
    Cygnus OB2, within the Cygnus X complex, is one of the most active star-forming regions of our Galaxy, hosting hundreds of O and B-type stars across different evolutionary stages. Despite extensive studies of its massive stars, Cygnus OB2 exhibits a notable absence of fast rotating stars (v sin i > 200 ), which challenges existing models of massive
    Galán-Diéguez, D. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Variability of star-forming galaxies around the SFMS and MZR
    The star-formation main sequence (SFMS) and the mass-metallicity relation (MZR) are two tight, fundamental relations that govern galaxy evolution. Their intrinsic scatter originates from some galaxies having above- or below-average SFR and metallicity, which leads to the question of whether galaxies which are offset from the relations stay there
    Camps-Fariña, A. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0